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scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

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STP12 Abstracts<br />

Berlin, 12 - 16 July <strong>2010</strong><br />

SCOSTEP Symposium <strong>2010</strong><br />

About existence of physical boundaries between structures of one polarity on the Sun.<br />

Ishkov Vitaly<br />

IIZMIRAN<br />

To one of the basic consequences active regions complexes (CAR) studying became opening<br />

existence of boundaries between magnetic "unipolar" structures of the same polarity. These<br />

boundaries are not defined on magnetogram received at observations of AR. Such bor<strong>der</strong>s<br />

inside of active regions c<strong>an</strong> be revealed at studying the dynamic phenomena, especially in<br />

flare processes. These boundaries, in case of realization of large solar flares, interfered with<br />

propagation of Hα flare emission to penetrates in the neighboring area. On <strong>an</strong> example of the<br />

large solar flare in AR3804 on July, 12th, 1982 it is possible to see, that the emission ribbon<br />

of N-polarity even during a maximum of flare does not penetration into areas of active region<br />

laying to the north of some boundaries.. The second example gives us active region AR4263<br />

on August - September, 1983 in which such boundaries passed between two space closely<br />

spots of one polarity. Umbra of spots all over again settled down in one penumbra, <strong>an</strong>d then<br />

dispatch noticeably, <strong>an</strong>d more east umbra, was noticeably turned counter-clockwise. If both<br />

umbra were in one "unipolar" structure (one system), should turn there were both umbra,<br />

however the physical bor<strong>der</strong> which is passed between spots, interfered with it. At the <strong>an</strong>alysis<br />

of the flares occurred in these AR, their spatial independence is well looked through: emission<br />

of flares carried out in one system un<strong>der</strong> no circumst<strong>an</strong>ces does not get into <strong>an</strong>other. The<br />

mo<strong>der</strong>n <strong>an</strong>alysis shows, that coronal holes arise just in a place of “physical” boundaries<br />

existence. From this point of view it is possible to assume that coronal holes are always<br />

formed in unipolar magnetic structures when such structures consist of two magnetic areas of<br />

one sign, but various origin <strong>an</strong>d between them necessarily there is a "physical" boundaries. In<br />

the solar corona where electrodynamic forces are weakened, there is a pushing away of these<br />

parts from each other <strong>an</strong>d magnetic field lines appear opened in interpl<strong>an</strong>etary space.

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